Published December 23, 2020
| Version v1
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Response curves butterfly filtering in LIGO O2
Description
Response curves in butterfly filtering to descending chirps in LIGO O2, calibrating output of chi-image analysis of merged (H1,L1)-spectrograms versus injection energies in Extended Emission to GW170817 (distance of 40Mpc). Response curves are shown for characteristic time-scales of frequency descent over 0.5-4.5 seconds for injection energies 0-8%MSolar c2. Results are averaged following times slides -10ms < Delta t < 10ms (light travel-time between the LIGO H1 and L1 detectors) and over three injection sites (one shown in first movie, closest to GW170817EE; all three shown in second movie).
Notes
Preferred citation: Central engine of GRB170817A: Neutron star versus Kerr black hole based on multimessenger calorimetry and event timing, Maurice H. P. M. van Putten, Massimo Della Valle A&A 669 A36 (2023), DOI: 10.1051/0004-6361/202142974
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- Video/Audio: https://zenodo.org/record/3544143 (URL)
- Is cited by
- Journal article: 10.1051/0004-6361/202142974 (DOI)